Le Corre, L.; Reddy, V.; Nathues, A.: Spectral Indices for Identifying Terrains on Vesta with Dawn Framing Camera Filters. Meteorit. Planet. Sci. 46, p. A135 - A135 (2011)
Le Corre, L.; Reddy, V.; Nathues, A.; Cloutis, E. A.: How to characterize terrains on 4 Vesta using Dawn Framing Camera color bands? Icarus 216 (2), pp. 376 - 386 (2011)
Reddy, V.; Nathues, A.; Gaffey, M. J.; Schaeff, S.: Mineralogical characterization of potential targets for the ASTEX mission scenario. Planetary and Space Science 59 (8), pp. 772 - 778 (2011)
Li, J.-Y.; Le Corre, L.; Reddy, V.; Nathues, A.; Hoffmann, M.; Schaefer, M.; Ciarniello, M.; Mottola, S.; Schröder, S. E.; Raymond, C. A.et al.; Russell, C. T.: Spectrophotometric Modeling and Mapping of Ceres. European Geosciences Union General Assembly, Vienna, Austria (2016)
Li, J.-Y.; Le Corre, L.; Reddy, V.; Nathues, A.; Hoffmann, M.; Schaefer, M.; Ciarniello, M.; Mottola, S.; Schröder, S. E.; Raymond, C. A.et al.; Russell, C. T.: Spectrophotometric Modeling and Mapping of Ceres. 47th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2016)
Schmidt, B. E.; Hughson, K. G.; Chilton, H. T.; Scully, J. E. C.; Platz, T.; Nathues, A.; Sizemore, H.; Bland, M. T.; Byrne, S.; Marchi, S.et al.; O'Brien, D. P.; Schorghofer, N.; Hiesinger, H.; Jaumann, R.; Lawrence, J.; Buczkowski, D.; Castillo, J. C.; Schenk, P. M.; Sykes, M. V.; De Sanctis, M. C.; Mitri, G.; Formisano, M.; Li, J.-Y.; Reddy, V.; LeCorre, L.; Russell, C. T.; Raymond, C. A.; the Dawn Science and Operations Team: Ground Ice on Ceres? 47th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2016)
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
The Sun’s planets and small objects have undergone substantial evolution. Deciphering the history of our cosmic home is not a simple task even though we now have access to a multitude of data gathered by space missions, remote observations, and laboratory studies of diverse samples. A significant fraction of materials available for the study of planetary bodies come from meteorites.